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The Spectral Schwartz Distribution
Wilhelm von Waldenfels
The spectral Schwartz distribution is connected with
the spectral measure, but it is in some way more gen-
eral and in some way more restricted than the spectral
measure. After the definition of the spectral Schwartz
distribution and some properties we present some ex-
amples. We calculate the resolvents of some operators
with the help of Krein’s formula and calculate then the
spectral Schwartz distribution. The method, how to
do this, has been developed by Gariy Efimov and my-
self in 1995 in a paper about radiation transfer. But the
method is so obvious, that it could be known before.
Assume we have a Banach space V and denote by L(V )
the space of all bounded linear operators from V to V
provided with the usual operator norm, and an open set
G ⊂ C and a function R(z) : G → L(V ) satisfying the
resolvent equation
R(z1)−R(z2) = (z2 − z1)R(z1)R(z2)..
The function R(z) is holomorphic in G. The subspace
D = R(z)V
is a subset independent of z ∈ G. If R(z0) is injective
for one z0 ∈ G, then R(z) is injective for all z ∈ G and
there exists a mapping a : D → V such that
(z − a)R(z)f = f for f ∈ VR(z)(z − a)f = f for f ∈ D
or
R(z) = (z − a)−1
and
aR(z) = −1 + zR(z) ; R(z)a = −1 + zR(z).
The operator a is closed and R(z) is the resolvent of a.
If G ⊂ C is open and f : G → C, f(z) = f(x + iy) has a
continuous derivative, set
∂f =df
dz=
1
2
(∂f
∂x− i
∂f
∂y
)∂f =
df
dz=
1
2
(∂f
∂x+ i
∂f
∂y
).
The function f is holomorphic if and only if ∂f = 0.
In an analogous way one defines these derivatives for
Schwartz distributions.
The function z 7→ 1/z is locally integrable and one ob-
tains
∂(1/z) = πδ(z).
Assume f to be defined and holomorphic for the ele-ments x+ iy ∈ G, y 6= 0, and that f(x± i0) exists, then
∂f(x+ iy) = (i/2)(f(x+ i0)− f(x− i0))δ(y)
Proposition Assume a function R(z) : G → L(V ), de-fined and obeying the resolvent equation almost every-where and a subspace V0 ⊂ V such that z 7→ (f |R(z)|g)is locally integrable for all f, g ∈ V0 then
z1, z2 7→ (f |R(z1)R(z2)|g)
is also locally integrable as well and for the Schwartzderivatives one has the formula
∂1∂2(f |R(z1)R(z2)|g) = πδ(z1 − z2)∂(f |R(z1)|g)
Definition Under the assumptions of the last proposi-
tion we call
M = (1/π)∂R
defined scalarly for f, g ∈ V0 by
(f |M(z)|g) = (1/π)∂(f |R(z)|g)
the spectral Schwartz distribution of R.
Under the assumptions of the last proposition and under
the additional assumption, that R(z) is injective, denote
again by a the operator defined by the resolvent. Then
we have
aM(z) = zM(z)
or more precisely
(f |aM(z)|g) = z(f |M(z)|g).
We consider again a function z ∈ G 7→ R(z) obeyingthe resolvent equation with values in a Hilbert spaceV and assume z, z ∈ G,=z 6= 0, R(z)∗ = R(z) and R(z)injective, and that D = R(z)V is dense in V . Then R(z)an be extended to the set of all z with =z 6= 0. If z 7→(f |R(z)|g), for f, g ∈ V0, is locally integrable, then thereexists a positive measure µ on R with values in L(V )defined by the sesquilinear forms f, g ∈ V0 7→ (f |µ(x)|g),such that
(f |M(x+ iy)|g) = (f |µ(x)|g)δ(y).
and
(f |µ(x)|g) =1
2πi(f |(R(x− i0)−R(x+ i0)|g)
Example 1 Suppose we have a matrix A with only
single eigenvalues and with the resolvent
R(z) =1
z −A=∑i
1
z − λipi
where pi are the eigenprojectors, so that pipj = piδij.
Then
M(z) = (1/π)∂R(z) =∑i
δ(z − λi)pi.
The last equation also holds if A is nilpotent, e.g., A2 =
0. Then one has to take
R(z) =1
z+A
Pz2,
where P denotes the principal value. Then
M(z) = δ(z)−A∂δ(z).
Example 2. Consider the multiplication operator Ω in
L2(R), given by (Ωf)(ω) = ωf(ω). The resolvent
RΩ(z) = (z −Ω)−1
is holomorphic outside the real line. The domain of Ω is
the space D = RΩ(z)L2, the space of all L2 functions f ,
such that Ωf is square integrable. Here we have defined
Ωf for all functions in a natural way. For f, g ∈ C1c
(f |RΩ(x± i0)|g) =∫
dωf(ω)g(ω)P/(x−ω)∓ iπf(x)g(x).
So so
(f |µ(x)|g) = f(x)g(x).
The the generalized eigen functions are
δx(ω) = δ(x− ω).
Using the formalism of bra and ket vectors we obtain
µ(x) = |δx)(δx|.
We have
RΩ(z) =∫
dx1
z − xµ(x) =
∫dx
1
z − x|δx)(δx|.
We have
Ω|δx) = x|δx).
The eigenvectors δx form a generalized orthonormal ba-
sis,i.e.
(δx|δy) = δ(x− y)∫
dx|δx)(δx| = 1.
The first equation ( orthonormality)can be checked di-rectly . The second equation (completeness) says, that∫
dxµ(x) = 1.
Example 3(Quantum probability:The pure number pro-cess) We consider the function R(z) which obeys theresolvent equation.
R(z) = RΩ(z) +1
1 + iπσ(z)RΩ(z)|E〉〈E|RΩ(z)
with σ(z) = signum = z and E is the constant functionE(ω) = 1 The expression
RΩ(z)|E〉 : RΩ(z)|E〉(ω) = 1/(z − ω)
is well defined in L2 and
〈E|RΩ(z) = RΩ(z)|E〉
In order to formulate the operator H corresponding to
R(z) we define the subspace L ⊂ L2
L = f = RΩ(z)(cE + f) : f ∈ L2
or more explicitely f ∈ L iff
f(ω) =1
z − ω(c+ f(ω))
Call L† the set of all semilinear functionals L → C. A
semilinear functional ϕ is additiv and ϕ(cf) = cϕ(f) for
f ∈ C. By the scalar product 〈g|f〉 =∫
dωg(ω)f(ω) we
associate to any f ∈ L2 a semilinear functional ϕ on L,
ϕ(ξ) = 〈ξ|f〉
As L is dense in L2 the functional determines f . So we
may imbed L2 into L† and
L ⊂ L2 ⊂ L†.
Define the functionals 〈E| ∈ L∗ and also |E〉 ∈ L† by
〈E|f〉 = limr→∞
∫ r−rf(ω)dω = −iπcσ(z) +
∫ 1
z − ωf(ω)dω
and
〈f |E〉 = 〈E|f〉.
Define the operator
Ω : L→ L†
〈g|Ωf〉 = limr→∞
∫ r−r
dωg(ω)ωf(ω)
Ωf = −c|E〉 − f + zf.
The domain of the selfadjoint operator H is
D = R(z)H =
RΩ(z)(|f〉+
(E|RΩ(z)|f〉1 + iσ(z)π
|E〉 : f ∈ L2⊂ L
The Hamiltonian H is the restriction of
H = Ω + |E〉〈E|
to that domain. With the methods used before we
calculate
M(x+ iy) = µ(x)δ(y)
µ(x) =1
2πi(R(x− i0)−R(x+ i0)) = |αx〉〈αx|
|αx〉 = (1 + π2)−1/2( Px−Ω
|E〉+ |δx〉)
. The αx form a generalized orthonormal basis in L2.
Example 4(Quantum probability: The Heisenberg equa-tion of the amplified oscillator) The underlying Hilbertspace is
H = C⊕ L2(R)
with the scalar product
〈(c, f)|(c′, g)〉 = cc′+∫
dxf(x)g(x).
We consider the function
R(z) =
(0 00 RΩ(z)
)+
(1
−RΩ(z)|E)
)1
z − iπσ(z)(1, (E|RΩ(z)) .
Define the operator
H : C⊕ L → C⊕ L†
H =
(0 (E|−|E) Ω
),
We have to distinguish between right and left domain
Dl resp Dr of the operator H corresponding to R(z).
Dl = HR(z) =
ξ ∈ C⊕ L : ξ = c(1, (E|R(z)) + (0, (f |)
Dr = R(z)H =
ξ ∈ C⊕ L : ξ = c
( 1
−R(z)|E)
)+( 0
R(z)f
)
with c ∈ C, f ∈ L2. The Hamiltonian H is the restriction
of H to Dl resp. Dr.
. The matrix H is not symmetric but it obeys to the
equation
JHJ = H+
with
J =
(−1 00 1
)
The resolvent R(z) is holomorphic outside the real line
and the two simple poles ±iπ. The spectral Schwartz
distribution M(z) = (1/π)∂R(z) has the form
M(x+ iy) = µ(x)δ(y) + p iπδ(z − iπ) + p− iπδ(z + iπ)
with
µ(x) =1
2πi(R(x− i0)−R(x+ i0)) = |αx〉〈βx|
|αx〉 = (x2 + π2)−1/2
( 1
− Px−Ω|E〉
)+ x
( 0
|δx〉
)〈βx| = (x2 + π2)−1/2
(− (1, 〈E|
Px−Ω
) + x(0, 〈δx|))
and
p±iπ = |α±iπ〉〈β±iπ| |α±iπ〉 =( 1
−1
±iπ −Ω|E〉
)
〈β±iπ| = (1, 〈E|1
±iπ −Ω)
It is easy to check the biorthonormality relations
〈αx|βy〉 = δ(x− y)
〈αx|β±iπ〉 = 0 (α±iπ|βx〉 = 0
〈α± iπ|β±iπ〉 = 1 α± iπ|β∓iπ〉 = 0
and completeness ∫dzM(z) = 1.
Example 5(Radiation transfer:grey atmosphere) De-
note
B = k ∈ R : |k| ≥ 1
and consider the operator
A = D − |η)(χ|
where D is the multiplication operator.
Df(k) = kf(k)
η(k) = sign(k)|k|−1/2
χ(k) = 12|k|−1/2
The operator can be defined by the resolvent
R(z) =1
z −D−
1
z −D|η)
PC(z)
(χ|1
z −Dwith
C(z) = 1 + (χ|1
z −D|η).
Near the origin
C(z) = −(χ|D−3|η)z2 + · · · = −13z
2 + · · · .
This necesssitates the introduction of P. The spectrumconsists of B and the origin, where we have a double
pole. For x ∈ B
C(x+i0) = 1+(χ|P
x−D−iπ(χ|δx)(δx|η) = CR(x)−iπCI(x).
We obtain
µ(x) = 1x ∈ B|αx)(βx|+ p0δ(x)− a0δ′(x).
with
|αx) = (C2R + π2C2
I )−1/2(CR|δx)−
Px−D
|η)(χ|δx)
)
(β| = (C2R + π2C2
I )−1/2(CR(δx| − (δx|η)(χ|
Px−D
)
p0 = (χ|D−3|η)−1(D−2|η)(χ|D−1 + (D−1|η)(χ|D−2
)
a0 = (χ|D−3|η)−1(D−1|η)(χ|D−1
)
Literature
G.V.Efimov, W.v.W.,R.Wehrse 1994
v.W.2013